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Article Contents

ABSTRACT

1.1.INTRODUCTORY REMARKS

1.2.CALIBRATION OF STAR FORMATION RATE INDICATORS ACROSS THE WAVELENGTH SPECTRUM
1.2.1.General characteristics
1.2.2.A word about the stellar initial mass function and stochastic sampling

1.3.THE NATURE OF `DIFFUSE' LIGHT IN GALAXIES

1.4.DUST ATTENUATION OF THE STELLAR LIGHT
1.4.1.General properties
1.4.2.Application to galaxies

1.5.LESSONS LEARNED
1.5.1.Global SFR indicators
1.5.2.Local SFR indicators

REFERENCES